Properties (50)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:aftermath |
remnant evolution studied over time
|
| gptkbp:analyzes |
data analysis revealed key characteristics
|
| gptkbp:associatedWith |
massive star collapse
|
| gptkbp:bombLoad |
approximately 1998
|
| gptkbp:collaborations |
involved multiple research institutions
|
| gptkbp:colors |
0.0055
|
| gptkbp:communityEngagement |
engaged with the astronomical community
|
| gptkbp:conservationEfforts |
remnant is still observable
|
| gptkbp:dataUsage |
data shared with global research community
data published in scientific journals |
| gptkbp:education |
has educational value for students and researchers
|
| gptkbp:established |
gptkb:Robert_Kirshner
|
| gptkbp:fuelType |
core-collapse supernova mechanism
|
| gptkbp:hasInternationalClassification |
classified as a Type II-P supernova
|
| gptkbp:hasRecognition |
initial magnitude of about -15.5
|
| gptkbp:historicalResearch |
collaborative research with international teams
|
| gptkbp:historicalSignificance |
historically significant for supernova research
|
| gptkbp:hosts |
NGC 3367
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1998bu
|
| gptkbp:image |
photometric data available in archives
|
| gptkbp:internationalClassification |
spectroscopy revealed presence of hydrogen
|
| gptkbp:legacy |
remains a legacy in supernova studies
|
| gptkbp:length |
approximately 24 million light-years from Earth
|
| gptkbp:lighting |
light curve fitting used to model explosion parameters
light curve lasted several months light curve shows a plateau phase plateau light curve reached peak brightness in May 1998 light curve analysis provided insights into explosion dynamics |
| gptkbp:lightRange |
light curve features analyzed for patterns
|
| gptkbp:locatedIn |
galaxy NGC 3367
|
| gptkbp:model |
theoretical models developed based on observations
|
| gptkbp:officialResidence |
data collected by various telescopes
observed over several years utilized various observational techniques |
| gptkbp:publicAccess |
generated public interest in astronomy
|
| gptkbp:realTimeTracking |
distance estimated using Tying method
|
| gptkbp:relatedEvent |
follow-up observations conducted for years after explosion
follow-up studies continue to this day |
| gptkbp:releaseYear |
1998-04-15
|
| gptkbp:researchInterest |
contributed to understanding of stellar evolution
|
| gptkbp:scientificName |
important for studying supernova mechanisms
|
| gptkbp:type |
Type II supernova
hydrogen-rich spectrum remnant classified as a supernova remnant |
| gptkbp:unitAwards |
maximum magnitude of about -17.5
|
| gptkbp:universe |
has implications for cosmology and distance measurements
|
| gptkbp:vision |
associated with a progenitor star of high mass
|
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|